Scalar self-energy for a charged particle in global monopole spacetime with a spherical boundary

被引:32
作者
Bezerra de Mello, E. R. [1 ]
Saharian, A. A. [1 ,2 ]
机构
[1] Univ Fed Paraiba, Dept Fis CCEN, BR-58059970 Joao Pessoa, Paraiba, Brazil
[2] Yerevan State Univ, Dept Phys, Yerevan 0025, Armenia
关键词
GRAVITATIONAL-FIELD; TIME; FORCE;
D O I
10.1088/0264-9381/29/13/135007
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We analyze combined effects of the geometry produced by a global monopole and a concentric spherical boundary on the self-energy of a point-like scalar charged test particle at rest. We assume that the boundary is outside the monopole's core with a general spherically symmetric inner structure. An important quantity to this analysis is the three-dimensional Green function associated with this system. For both Dirichlet and Neumann boundary conditions obeyed by the scalar field on the sphere, the Green function presents a structure that contains contributions due to the background geometry of the spacetime and the boundary. Consequently, the corresponding induced scalar self-energy also presents a similar structure. For points near the sphere, the boundary-induced part dominates and the self-force is repulsive/attractive with respect to the boundary for Dirichlet/Neumann boundary condition. In the region outside the sphere at large distances from it, the boundary-free part in the self-energy dominates and the corresponding self-force can be either attractive or repulsive with dependence of the curvature coupling parameter for scalar field. In particular, for the minimal coupling we show the presence of a stable equilibrium point for the Dirichlet boundary condition. In the region inside the sphere, the nature of the self-force depends on the specific model for the monopole's core. As illustrations of the general procedure adopted, we shall consider two distinct models, namely the flower-pot and the ballpoint-pen ones.
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页数:25
相关论文
共 37 条
[1]  
Abramowitz M., 1964, Handbook of Mathematical Functions
[2]   EFFECTS OF CURVATURE COUPLINGS FOR QUANTUM-FIELDS ON COSMIC-STRING SPACE-TIMES [J].
ALLEN, B ;
OTTEWILL, AC .
PHYSICAL REVIEW D, 1990, 42 (08) :2669-2677
[3]  
[Anonymous], 1967, Principles of Relativity Physics
[4]  
[Anonymous], SOV PHYS JETP
[5]   Induced self-energy on a static scalar charged particle in the spacetime of a global monopole with finite core [J].
Barbosa, D. ;
de Freitas, U. ;
Bezerra de Mello, E. R. .
CLASSICAL AND QUANTUM GRAVITY, 2011, 28 (06)
[6]   INDUCED ELECTROSTATIC SELF-INTERACTION IN THE SPACE-TIME OF A GLOBAL MONOPOLE WITH INNER STRUCTURE (vol 18, pg 1085, 2009) [J].
Barbosa, D. ;
Spinelly, J. ;
Bezerra De Mello, E. R. .
INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 2011, 20 (01) :119-120
[7]   INDUCED ELECTROSTATIC SELF-INTERACTION IN THE SPACE-TIME OF A GLOBAL MONOPOLE WITH INNER STRUCTURE [J].
Barbosa, D. ;
Bezerra De Mello, E. R. ;
Spinelly, J. .
INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 2009, 18 (07) :1085-1099
[8]   GRAVITATIONAL-FIELD OF A GLOBAL MONOPOLE [J].
BARRIOLA, M ;
VILENKIN, A .
PHYSICAL REVIEW LETTERS, 1989, 63 (04) :341-343
[9]   Vacuum polarization effects on flat branes due to a global monopole [J].
Bezerra de Mello, E. R. .
PHYSICAL REVIEW D, 2006, 73 (10)
[10]   Fermionic vacuum polarization in a higher-dimensional global monopole spacetime [J].
Bezerra de Mello, E. R. .
PHYSICAL REVIEW D, 2007, 76 (12)